Published on:
24 October 2023
Primary Category:
Cosmology and Nongalactic Astrophysics
Paper Authors:
Tian-Nuo Li,
Shang-Jie Jin,
Hai-Li Li,
Jing-Fei Zhang,
Xin Zhang
Gravitational waves from neutron star mergers can precisely measure cosmic expansion
But gravitational waves alone cannot tightly constrain dark matter-dark energy interaction
Combining gravitational waves with cosmic microwave background breaks degeneracies
Improves interaction strength constraints by 70% over current data
Results are not affected much by neutron star equation of state
Probing dark energy-dark matter interaction with gravitational waves
This paper investigates using gravitational waves from neutron star mergers to probe the interaction between dark energy and dark matter. Simulations show gravitational waves alone cannot tightly constrain interaction strength, but when combined with cosmic microwave background data, constraints improve significantly. Results are robust to different neutron star equations of state.
Measuring thermal effects in neutron star mergers
Gravitational wave detectors improve cosmological constraints
Dark matter interactions alter early universe
Dark energy effects on compact stars
Gravitational waves reveal neutron star structure
Gravitational waves reveal sound speed dips enabling primordial black holes
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